Search Publications

The anatomy of a wrinkle ridge revealed in the wall of Melas Chasma, Mars
DOI: 10.1002/2017JE005274 Bibcode: 2017JGRE..122..889C

Andrews-Hanna, Jeffrey C.; Cole, Hank M.

Wrinkle ridges are among the most common tectonic structures on the terrestrial planets and provide important records of the history of planetary strain and geodynamics. The observed broad arches and superposed narrow wrinkles are thought to be the surface manifestation of blind thrust faults, which terminate in near-surface volcanic sequences and…

2017 Journal of Geophysical Research (Planets)
MEx 12
Energy-angle dispersion of accelerated heavy ions at 67P/Churyumov-Gerasimenko: implication in the mass-loading mechanism
DOI: 10.1093/mnras/stx1621 Bibcode: 2017MNRAS.469S.339N

Yamauchi, M.; Behar, E.; Nilsson, H. +4 more

The Rosetta spacecraft studied the comet 67P/Churyumov-Gerasimenko for nearly two years. The Ion Composition Analyzer instrument on board Rosetta observed the positive ion distributions in the environment of the comet during the mission. A portion of the comet's neutral coma is expected to get ionized, depending on the comet's activity and positio…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 12
Primordial power spectrum features in phenomenological descriptions of inflation
DOI: 10.1016/j.dark.2017.07.003 Bibcode: 2017PDU....17...38G

Mena, Olga; Boubekeur, Lotfi; Gariazzo, Stefano +1 more

We extend an alternative, phenomenological approach to inflation by means of an equation of state and a sound speed, both of them functions of the number of e-folds and four phenomenological parameters. This approach captures a number of possible inflationary models, including those with non-canonical kinetic terms or scale-dependent non-gaussiani…

2017 Physics of the Dark Universe
Planck 12
Signatures of the Martian rotation parameters in the Doppler and range observables
DOI: 10.1016/j.pss.2017.05.008 Bibcode: 2017P&SS..144...74Y

Yseboodt, Marie; Dehant, Véronique; Péters, Marie-Julie

The position of a Martian lander is affected by different aspects of Mars' rotational motions: the nutations, the precession, the length-of-day variations and the polar motion. These various motions have a different signature in a Doppler observable between the Earth and a lander on Mars' surface. Knowing the correlations between these signatures …

2017 Planetary and Space Science
ExoMars-16 12
Post-flare formation of the accretion stream and a dip in pulse profiles of LMC X-4
DOI: 10.1016/j.newast.2017.05.001 Bibcode: 2017NewA...56...94B

Paul, Biswajit; Beri, Aru

We report here a pulse profile evolution study of an accreting X-ray pulsar LMC X-4 during and after the large X-ray flares using data from the two observatories XMM-Newton and RXTE. During the flares, the pulse profiles were found to have a significant phase offset in the range of 0.2-0.5 compared to the pulse profiles immediately before or after…

2017 New Astronomy
XMM-Newton 12
Detection of Prominent Stellar Disks in the Progenitors of Present-day Massive Elliptical Galaxies
DOI: 10.3847/1538-4357/836/1/75 Bibcode: 2017ApJ...836...75D

Ho, Luis C.; Mobasher, Bahram; Canalizo, Gabriela +1 more

Massive galaxies at high redshifts (z > 2) show different characteristics from their local counterparts: they are compact and most likely have a disk. In this study, we trace the evolution of local massive galaxies by performing a detailed morphological analysis, namely, fitting single Sérsic profiles and performing bulge+disk decompositions. W…

2017 The Astrophysical Journal
eHST 12
CTIO, ROSAT HRI, and Chandra ACIS Observations of the Archetypical Mixed-morphology Supernova Remnant W28 (G6.4-0.1)
DOI: 10.3847/1538-4357/aa615c Bibcode: 2017ApJ...839...59P

Kargaltsev, Oleg; Rho, Jeonghee; Hare, Jeremy +6 more

We present a joint analysis of optical emission-line and X-ray observations of the archetypical Galactic mixed-morphology supernova remnant (MMSNR) W28 (G6.4-0.1). MMSNRs comprise a class of sources whose shell-like radio morphology contrasts with a filled center in X-rays; the origin of these contrasting morphologies remains uncertain. Our CTIO i…

2017 The Astrophysical Journal
XMM-Newton 12
The effect of unresolved contaminant stars on the cross-matching of photometric catalogues
DOI: 10.1093/mnras/stx629 Bibcode: 2017MNRAS.468.2517W

Wilson, Tom J.; Naylor, Tim

A fundamental process in astrophysics is the matching of two photometric catalogues. It is crucial that the correct objects be paired, and that their photometry does not suffer from any spurious additional flux. We compare the positions of sources in Wide-field Infrared Survey Explorer (WISE), INT Photometric H α Survey, Two Micron All Sky Survey …

2017 Monthly Notices of the Royal Astronomical Society
Gaia 12
Multi-spacecraft Observations of the Coronal and Interplanetary Evolution of a Solar Eruption Associated with Two Active Regions
DOI: 10.3847/1538-4357/aa6d54 Bibcode: 2017ApJ...840...76H

Wang, Rui; Yang, Zhongwei; Liu, Ying D. +3 more

We investigate the coronal and interplanetary evolution of a coronal mass ejection (CME) launched on 2010 September 4 from a source region linking two active regions (ARs), 11101 and 11103, using extreme ultraviolet imaging, magnetogram, white-light, and in situ observations from SDO, STEREO, SOHO, VEX, and Wind. A potential-field source-surface m…

2017 The Astrophysical Journal
SOHO VenusExpress 12
Simulated Galactic methanol maser distribution to constrain Milky Way parameters
DOI: 10.1051/0004-6361/201730681 Bibcode: 2017A&A...604A..72Q

Reid, M. J.; Quiroga-Nuñez, L. H.; van Langevelde, H. J. +1 more

Context. Using trigonometric parallaxes and proper motions of masers associated with massive young stars, the Bar and Spiral Structure Legacy (BeSSeL) survey has reported the most accurate values of the Galactic parameters so far. The determination of these parameters with high accuracy has a widespread impact on Galactic and extragalactic measure…

2017 Astronomy and Astrophysics
Gaia 12